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Characterizing the heavy elements in globular cluster M22 and an empirical s-process abundance distribution derived from the two stellar groups

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http://pubman.mpdl.mpg.de/cone/persons/resource/persons26329

Marino,  A. F.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Roederer, I. U., Marino, A. F., & Sneden, C. (2011). Characterizing the heavy elements in globular cluster M22 and an empirical s-process abundance distribution derived from the two stellar groups. The Astrophysical Journal, 742(1): 37, pp. 1-16. doi:10.1088/0004-637X/742/1/37.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000F-3A78-B
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